DIRECT MEASUREMENTS OF THE GENERAL MAGNETIC FIELD ON THE SOLAR-LIKE STARS

Автор(и)

  • S. I. Plachinda Crimean Astrophysical Observatory and Isaac Newton Institute of Chile, Crimean Branch, Nauchny, 98409 Crimea, Ukraine, Україна
  • C. M. Johns-Krull Space Sciences Laboratory, University of California, Berkeley, CA 94720-7450 USA, США
  • T. N. Tarasova Crimean Astrophysical Observatory and Isaac Newton Institute of Chile, Crimean Branch, Nauchny, 98409 Crimea, Ukraine, Україна

DOI:

https://doi.org/10.18524/1810-4215.2001.14.99480

Ключові слова:

Stars, late-type, stars, individual, 61 Cyg A, &xi, Boo A, Sun, magnetic fields.

Анотація

We report the high-precision spectropolarimetric measurements of the general magnetic field (GMF) on a solar-like star 61 Cyg A. The magnetic field shows periodic variations due to stellar rotation with a period of Pmf = 36.59 ± 0.18 days. The net longitudinal magnetic field of 61 Cyg A varied from –13 G to + 4 G. The conclusion was made that the nonaxisymmetric large-scale magnetic field (original magnetic field - OMF) on the surface of the Sun and solar-like stars ξ Boo A and 61 Cyg A is present in addition to toroidal and axisymmetric poloidal fields, which are produced by dynamo. The characteristics of the OMF point to a presence of a global magnetic field in the star radiative interior and re internal field properties on the surface. The birth and formation of magnetic active regions (ARs) on the surface of the solar-like star 61 Cyg A has been registered. The numerical simulations were compared with magnetic measurements, and lead us to the conclusion about the presence on 61 Cyg A of more strong magnetic of ARs (∼ 1023 – 1024 Mx) than on the Sun. These ARs can be formed at the same latitudes as on the Sun.

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Опубліковано

2017-04-20

Номер

Том 14 (2001)

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